High Resolution Multislit Spectroscopy of Solar Corona in two lines during the Total Solar Eclipse of Oct. 24, 1995

dc.contributor.author	Singh, J
dc.contributor.author	Gupta, S. S
dc.contributor.author	Cowsik, R
dc.date.accessioned	2005-01-17T11:14:41Z
dc.date.available	2005-01-17T11:14:41Z
dc.date.issued	1997
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 13, pp. 47-51	en
dc.identifier.issn	0374-3632
dc.identifier.uri	http://hdl.handle.net/2248/239
dc.description.abstract	Two coronal emission lines 5303 Armstrong (Fe XIV) and 6374 Armstrong (Fe X) corresponding to ionization temperatuess of 2 and 1 million degree kelvin respectively were used to obtain the high resolution coronal spectra using multislit spectrograph. The experimental setup provided a spatial resolution of 11 arcsec and spectral resolution of 70 mA corresponding to a velocity of about 4 Kms(-1). The spectra were recorded on 70mm kodak 4415 film using Hamamatsu image intensifiers. For the first time we were able to obtain the high resolution spectra in these two emission lines simultaneously at various locations in the solar corona.	en
dc.format.extent	277489 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Coronal temperature	en
dc.subject	Emission lines	en
dc.subject	Ionization and kinetic temperatures	en
dc.subject	Turbulence	en
dc.title	High Resolution Multislit Spectroscopy of Solar Corona in two lines during the Total Solar Eclipse of Oct. 24, 1995	en
dc.type	Article	en